TY  - GEN 
AU  - Van der Giessen, S. A.
PY  - 2022
UR  - http://hdl.handle.net/10481/75708
AB  - Attenuation by dust severely impacts our ability to obtain unbiased observations of galaxies, especially as the amount and wavelength dependence of the attenuation varies with the stellar mass M-, inclination i, and other galaxy properties. In this...
LA  - eng
PB  - EDP
KW  - Galaxies: star formation
KW  - Ultraviolet: galaxies
KW  - Galaxies: evolution
KW  - Galaxies: ISM
KW  - Dust, extinction
TI  - Probing star formation and ISM properties using galaxy disk inclination. III. Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
DO  - 10.1051/0004-6361/202142452
ER  -